The Broad Line Region in Active Galactic Nuclei

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dc.creatorDultzin-Hacyan, D.
dc.creatorMarziani, P.
dc.creatorSulentic, J. W.
dc.date2000-02-04
dc.date.accessioned2026-07-07T01:52:07Z
dc.date.available2026-07-07T01:52:07Z
dc.descriptionWe review constraints on models of the broad line region that are imposed by observations of the emission lines in Active Galactic Nuclei. Comparison of high and low ionization lines in sources with FWHM Hbeta < 4000 km/s points toward low ionization line emission produced in a flattened geometry (the accretion disk?) with an associated high ionization wind. It remains unclear whether these results can be extended to all radio quiet AGN and particularly to radio loud AGN.
dc.description8 pages, 2 figures. Invited talk to be published in Astrophysical Plasmas: Codes, Models and Observations, proceedings of a meeting held on October 25--29, 1999 at Mexico City, Rev. Mexicana de Astron. y Astrof., Serie de Conferencias
dc.identifierhttps://arxiv.org/abs/astro-ph/0002096
dc.identifierhttp://arxiv.org/abs/astro-ph/0002096
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/513
dc.subjectAstrophysics
dc.titleThe Broad Line Region in Active Galactic Nuclei
dc.typetext

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